Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass

Fuente: arXiv
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Autori principali: Gonçalves, João, Marfatia, Danny, Morais, António P., Pasechnik, Roman
Natura: Preprint
Pubblicazione: 2024
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author Gonçalves, João
Marfatia, Danny
Morais, António P.
Pasechnik, Roman
author_facet Gonçalves, João
Marfatia, Danny
Morais, António P.
Pasechnik, Roman
contents We study supercooled first-order phase transitions above the QCD scale in a wide class of conformal Majoron-like U(1)' models that explain the totality of active neutrino oscillation data and produce a detectable stochastic gravitational wave background (SGWB) at LIGO, LISA and ET. We place constraints on the U(1)' breaking scale and gauge coupling using current LIGO-Virgo-Kagra data. We find that strong supercooling can be ruled out in large regions of parameter space if a SGWB is not detected by these experiments. A null signal at LIGO and ET will disfavor a type-I seesaw scale above $10^{14}$ GeV, while a positive signal is a signature of heavy right-handed neutrinos. On the other hand, LISA will be sensitive to seesaw scales as low as a TeV, and could detect a SGWB even if the right-handed neutrinos are decoupled.
format Preprint
id arxiv_https___arxiv_org_abs_2412_02645
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass
Gonçalves, João
Marfatia, Danny
Morais, António P.
Pasechnik, Roman
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Experiment
We study supercooled first-order phase transitions above the QCD scale in a wide class of conformal Majoron-like U(1)' models that explain the totality of active neutrino oscillation data and produce a detectable stochastic gravitational wave background (SGWB) at LIGO, LISA and ET. We place constraints on the U(1)' breaking scale and gauge coupling using current LIGO-Virgo-Kagra data. We find that strong supercooling can be ruled out in large regions of parameter space if a SGWB is not detected by these experiments. A null signal at LIGO and ET will disfavor a type-I seesaw scale above $10^{14}$ GeV, while a positive signal is a signature of heavy right-handed neutrinos. On the other hand, LISA will be sensitive to seesaw scales as low as a TeV, and could detect a SGWB even if the right-handed neutrinos are decoupled.
title Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Experiment
url https://arxiv.org/abs/2412.02645